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dc.contributor.authorOgura, Yoshimitsu
dc.date.accessioned2017-06-09T14:12:01Z
dc.date.available2017-06-09T14:12:01Z
dc.date.copyright1958/12/01
dc.date.issued1958
dc.identifier.issn0095-9634
dc.identifier.otherams-14479.pdf
dc.identifier.urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150044
dc.description.abstractAn attempt is made to see what the results of the application of the methods of Heisenberg are to isotropic temperature fluctuations in a stationary isotropic turbulence, under the restriction that temperature differences are too small to have any effect on the velocity field. The power spectrum for temperature fluctuations, thus deduced, degenerates to those obtained previously by Corrsin at two extremes-i.e., in intermediate and highest wave number ranges. The shape of the correlation function is also derived and compared with the experimental results of Shiotani. Finally, the thermal microscale and the size of the smallest eddies are expressed in terms of the turbulent Reynolds number and Péclet number or the fluid Prandtl number.
dc.publisherAmerican Meteorological Society
dc.titleTEMPERATURE FLUCTUATIONS IN AN ISOTROPIC TURBULENT FLOW
dc.typeJournal Paper
dc.journal.volume15
dc.journal.issue6
dc.journal.titleJournal of Meteorology
dc.identifier.doi10.1175/1520-0469(1958)015<0539:TFIAIT>2.0.CO;2
dc.journal.fristpage539
dc.journal.lastpage546
dc.treeJournal of Meteorology:;1958:;volume( 015 ):;issue: 006
dc.contenttypeFulltext


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